{"version":3,"sources":["webpack:///./src/data/phenomena/zh/earth-magnetosphere.md"],"names":["module","exports","body","html","attributes","vue","render","staticRenderFns","component","data","templateRender","createElement","this","created","_vm","_h","$createElement","_self","_c","_m","$options","staticClass","_v","attrs","src","alt","href","controls","type"],"mappings":"mGAAAA,EAAAC,QAAA,CACAC,KAAA,miBACAC,KAAA,ypBACAC,WAAA,GACAC,IAAA,CACAC,OAAA,+GACAC,gBAAA,4oCACAC,UAAA,CACAC,KAAA,WACA,OACAC,eAAA,OAGAJ,OAAA,SAAAK,GACA,OAAAC,KAAAF,eAAAE,KAAAF,iBAAAC,EAAA,oBAEAE,QAAA,WACAD,KAAAF,eAAA,WAAqD,IAAAI,EAAAF,KAAcG,EAAAD,EAAAE,eAA0BF,EAAAG,MAAAC,GAAwB,OAAAJ,EAAAK,GAAA,IACrHP,KAAAQ,SAAAb,gBAAA,YAA0D,IAAAO,EAAAF,KAAcG,EAAAD,EAAAE,eAA0BE,EAAAJ,EAAAG,MAAAC,IAAAH,EAAwB,OAAAG,EAAA,OAAiBG,YAAA,iBAA4B,CAAAH,EAAA,MAAAJ,EAAAQ,GAAA,UAAAR,EAAAQ,GAAA,KAAAJ,EAAA,KAAAA,EAAA,OAA0DK,MAAA,CAAOC,IAAA,4BAAAC,IAAA,mBAAyDX,EAAAQ,GAAA,KAAAJ,EAAA,MAAAJ,EAAAQ,GAAA,iBAAAR,EAAAQ,GAAA,KAAAJ,EAAA,KAAAJ,EAAAQ,GAAA,wBAAAJ,EAAA,UAAAJ,EAAAQ,GAAA,QAAAR,EAAAQ,GAAA,QAAAJ,EAAA,KAAqJK,MAAA,CAAOG,KAAA,6BAAmC,CAAAZ,EAAAQ,GAAA,SAAAR,EAAAQ,GAAA,sCAAAJ,EAAA,UAAAJ,EAAAQ,GAAA,WAAAR,EAAAQ,GAAA,MAAAJ,EAAA,UAAAJ,EAAAQ,GAAA,UAAAR,EAAAQ,GAAA,2DAAAJ,EAAA,UAAAJ,EAAAQ,GAAA,SAAAR,EAAAQ,GAAA,yBAAAJ,EAAA,UAAAJ,EAAAQ,GAAA,QAAAR,EAAAQ,GAAA,OAAAR,EAAAQ,GAAA,KAAAJ,EAAA,KAAAJ,EAAAQ,GAAA,6CAAAR,EAAAQ,GAAA,KAAAJ,EAAA,SAAkZK,MAAA,CAAOI,SAAA,KAAe,CAAAT,EAAA,UAAeK,MAAA,CAAOC,IAAA,8BAAAI,KAAA,eAAwDd,EAAAQ,GAAA,sDAAAR,EAAAQ,GAAA,KAAAJ,EAAA,KAAAA,EAAA,MAAAJ,EAAAQ,GAAA","file":"js/chunk-2d0e64ff.5189c3c6.js","sourcesContent":["module.exports = { \n body: \"# 地球磁層\\n\\n![Magnetosphere](./static/earth_mag_ch.png)\\n*(來源︰NASA)*\\n\\n地球核心中熔化鐵的流動產生電流,從而產生**磁場**。透過與太陽風的相互作用,這磁場形成一地球的屏障,稱為磁層。磁層保護我們免受太陽的**紫外線輻射**以及**宇宙輻射**(太空中無處不在的高能粒子)影響。帶電粒子撞擊屏障(磁層)時不會直接進入地球表面,而會流向周圍,並困於一個稱為**輻射帶**的區域 。其中有一部分會跟隨磁場向下移動到**極地**。\\n\\n太陽風為地球磁場帶來的壓力會壓縮地球磁場向日的一側,並拉長地球磁場背日的一側。\\n\\n\\n\\n*這動畫顯示日冕物質拋射如何從太陽放出,並干擾地球的磁場(彎曲的紫色線),因而產生極光(環繞北極和南極的藍色光環)。(來源: 美國太空總署)*\\n\",\n html: \"

地球磁層

\\n

\\\"Magnetosphere\\\"\\n(來源︰NASA)

\\n

地球核心中熔化鐵的流動產生電流,從而產生磁場。透過與太陽風的相互作用,這磁場形成一地球的屏障,稱為磁層。磁層保護我們免受太陽的紫外線輻射以及宇宙輻射(太空中無處不在的高能粒子)影響。帶電粒子撞擊屏障(磁層)時不會直接進入地球表面,而會流向周圍,並困於一個稱為輻射帶的區域 。其中有一部分會跟隨磁場向下移動到極地

\\n

太陽風為地球磁場帶來的壓力會壓縮地球磁場向日的一側,並拉長地球磁場背日的一側。

\\n\\n

這動畫顯示日冕物質拋射如何從太陽放出,並干擾地球的磁場(彎曲的紫色線),因而產生極光(環繞北極和南極的藍色光環)。(來源: 美國太空總署)

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